Replication data for:

A.P. Crósta, E.A. Silber, R.M.C. Lopes, B.C. Johnson, E. Bjonnes, M.J. Malaska, 
S.D. Vance, C. Sotin, A. Solomonidou, J.M. Soderblom (2021) Modeling the formation 
of Menrva impact crater on Titan: Implications for habitability, Icarus, 114679

https://doi.org/10.1016/j.icarus.2021.114679.
(https://www.sciencedirect.com/science/article/pii/S0019103521003365)
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This database contains .zip files* that represent simulated scenarios as described 
in the published text.
Each .zip file or the .zip file pair* (*_a.zip and *_b.zip) contains the following:
- material.inp (material input file)
- asteroid.inp (asteroid input file)
- jdata.dat (simulation output)

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File name structure:
	
titan_[X]km_ocean_[Y]km_lid[Z]km_[U]K.tar

X = projectile diameter
Y = thickness of the ice shell (or depth at which the liquid ocean begins)
Z = approximate thickness of the stagnant conductive lid
U = temperature of the warm convective ice

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*Due to the data file size limitation, some simulation outputs** (jdata.dat) are 
split into two files, 'jdata.dat.aa' and 'jdata.dat.ab'. These need to be combined 
before futher post-processing. 

Example how to combine the files on a Mac using terminal:

cat jdata.dat.aa jdata.dat.ab > jdata.dat

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** Scenarios where the projectile diameter is 34 km